We present a method to flexibly and self-consistently determine individual galaxies' star
formation rates (SFRs) from their host haloes' potential well depths, assembly histories, and …

We present a robust method to constrain average galaxy star formation rates (SFRs), star
formation histories (SFHs), and the intracluster light (ICL) as a function of halo mass. Our …

Satellite galaxies in groups and clusters are more likely to have low star formation rates
(SFRs) and lie on the 'red sequence'than central ('field') galaxies. Using galaxy group/cluster …

We have updated and extended our semi-analytic galaxy formation modelling capabilities
and applied them simultaneously to the stored halo/subhalo merger trees of the Millennium …

ABSTRACT Lambda Cold Dark Matter (ΛCDM) is now the standard theory of structure
formation in the universe. We present the first results from the new Bolshoi dissipationless …

The boundaries of cold dark matter halos are commonly defined to enclose a density
contrast Δ relative to a reference (mean or critical) density. We argue that a more physical …

We conduct a comprehensive analysis of the relationship between central galaxies and their
host dark matter halos, as characterized by the stellar mass–halo mass (SM–HM) relation …

Aims. Understanding the link between the galaxy properties and the dark matter halos they
reside in and their coevolution is a powerful tool for constraining the processes related to …

We measure the luminosity and color dependence of galaxy clustering in the largest-ever
galaxy redshift survey, the main galaxy sample of the Sloan Digital Sky Survey Seventh Data …

We use a statistical approach to determine the relationship between the stellar masses of
galaxies and the masses of the dark matter halos in which they reside. We obtain a …